Chapter 14: NMR Spectroscopy A. Introduction MS and IR can - - PDF document

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Chapter 14: NMR Spectroscopy

• A. Introduction
• MS and IR can provide MW and a few other details, but we

generally need way more info to fully determine a structure.

• Nuclear magnetic resonance (NMR) spectroscopy is a very

powerful technique for structure determination.

• 1H NMR (“proton NMR”) provides details about the number,

types, and relationships of H atoms in a molecule.

• 13C NMR provides details about the number and types of C

atoms in a molecule.

• NMR involves an effect on nuclei that occurs when molecules

are exposed to radiofrequency energy while in a magnetic field...

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All nuclei are charged, and have a spin quantum number (“I”) that can be 0, ½ , 1, etc. depending on the type of nucleus. If I ≠ 0, the nucleus has a net spin. For 1H, the value is ½. When a charged particle (like a 1H nucleus, i.e., a proton) spins, it creates a tiny magnetic field, making it like a tiny bar magnet. Normally, these are randomly oriented in space. However, in an external magnetic field (B0), they become aligned “with” or “against” this applied field.

• B. The NMR Effect

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• This creates two possible energy states for each 1H:

alignment with B0 is lower in energy, but only by a bit (< 0.1 cal), so the populations of the states are similar.

• If energy that matches the E between these two states is

applied, it is absorbed by lower energy nuclei, causing them to excite or “flip” to the higher E orientation.

• The value of E needed lies in the radiofrequency (RF) range.
• At the appropriate E for a given B0, such excitation occurs,

placing the nuclei in energetic “resonance” (not our usual definition of resonance…)

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• The stronger the B0 (in tesla; T) , the larger the E, and the higher

the RF energy needed for resonance (in megahertz; MHz).

• Very powerful (superconducting!) magnets are needed to create

large enough B0 (and E) to make the experiment most useful.

• NMR spectrometers are classified according to the RF energy

value needed for 1H resonance (e.g., 300 MHz, 500 MHz, etc.)

• The magnet strength (B0) is chosen to give these round

numbers, e.g., if B0 = 7.04 T, 1H frequency = 300 MHz

• C. Resonance Frequency

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• D. Chemical Shift
• A key element of the usefulness of NMR lies in the fact that

environmental differences cause slight differences in the exact frequencies at which individual nuclei resonate.

• This phenomenon is called “chemical shift” ().
• These differences are on the order of parts-per-million (ppm);

most 1H NMR absorptions appear within a 10 ppm window. Q: Why does the environment of a nucleus affect its resonating frequency? A: The e- nearby are also charged and affected by B0.

• Their circulation leads to a

contribution opposed to B0 (in the vicinity of the nucleus)

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• The H experiences a lower effective B, thereby increasing the

external B needed for resonance (to compensate) and increasing the frequency (E) needed, as well.

• Key, net result: The signal for the 1H is “shifted” to higher field.
• Magnitude of effect depends on e- density around the nucleus…
• As e- density increases, nuclei are said to become more shielded.

(Resonance frequency at higher magnetic field; more “upfield”).

• As e- density decreases, nuclei are increasingly deshielded.

(Resonance at lower field; further “downfield”).

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• e- density, in turn, depends on chemical environment (e.g.,

nearby functional groups, electronegativity of attached atoms,  e- density in the area, resonance effects, etc.) Consider these 3 examples (showing electronegativity effects): Hb’s have less e- density than Ha’s due to Cl → more deshielded → more downfield than Ha’s Hb’s have less e- density than Ha’s (F vs. Br) → more deshielded → more downfield than Ha’s Hb’s have less e- density than Ha’s (2 Cl vs. 1 Cl) → more deshielded → more downfield than Ha’s We’ve seen halide substituents reduce e- density before, e.g., recall the effects of replacing H’s with halides on pKa of CH3COOH…

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• E. A Modern NMR Spectrometer
• A pulse of energy is applied to a solution of a compound to

achieve simultaneous resonance of all its 1H’s.

• After this energy “pulse”, nuclei return to their equilibrium

distribution--the instrument detects the emitted energy to generate a spectrum that shows the individual “resonances”.

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• An NMR spectrum is a plot of peak intensity vs. chemical shift

() in ppm “downfield” relative to a standard reference (tetramethylsilane; TMS) set by convention as 0 ppm.

• TMS was chosen for many reasons, but because it is upfield of

most organics, shift numbers increase from right to left.

• F. 1H NMR Spectra

CH3OC(CH3)3

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• The chemical shift of an NMR resonance (or “signal”), in ppm,

is measured according to the following equation:

• Because shift of a signal is reported as a fraction (i.e., in ppm)
• f whatever NMR operating frequency is being used, it is a

constant for a given sample.

• However, in a 300-MHz (i.e., 300 million Hz) spectrum, 1 ppm =

300 Hz. In a 600-MHz spectrum, 1 ppm = 600 Hz.

• Thus, signals will be more spread out at 600-MHz, making

fortuitous, confusing overlap of different signals less likely.

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Superconducting magnets are really expensive, but this begins to explain why we care about going to higher frequencies… It improves both resolution of the signals and sensitivity. This is most important for real-world samples that are limited in quantity and/or have complex structures showing many signals.

8 7 6 5 4 3 2 1 PPM

N O H OH OCH3 O OH O O H

A 600-MHz 1H NMR spectrum of a more complex molecule:

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• Number of signals: indicates the number of “different types
• f H” (i.e., different environments of H’s) in a molecule.
• Position of signals: helps sort out what types of H the

molecule contains.

• Intensity (peak area) of signals: indicates the relative

amounts (how many) of each kind of H.

• Shape (spin-spin coupling/splitting/multiplicity) of a signal:

gives info about neighboring H’s in the molecule.

• G. Types of Structural Info Provided by 1H NMR Spectra

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• 1H’s in different environments give different NMR signals.
• 1H’s in equivalent environments collectively give one NMR signal.
• The number of signals equals the number of different types of 1H

in a compound (unless signals fortuitously overlap…).

• 1. Number of Signals

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• In comparing two H atoms on a C=C (or a ring…), two H’s are

equivalent only if they are cis (or trans) to the same groups.

• a. Alkenes—issues introduced by C=C geometry…
• This shows that it is possible for two H’s on the same C to be

different....

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• b. Substituted Cycloalkanes
• To determine whether two H’s in a cycloalkane (or an alkene)

are equivalent, consider whether or not the H’s in question are cis (or trans) to the same groups.

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• c. Enantiotopic Protons
• If Ha below were replaced by “Z”, we’d get a different

enantiomer than we would if Hb were replaced by Z.

• These two H’s are considered enantiotopic, and are chemical-

shift equivalent (i.e., they will give one 1H NMR signal).

• It may seem obvious that two H’s on the same sp3 C would be

equivalent, but look at the next case…

(Note that this molecule is achiral)

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• d. Diastereotopic Protons
• If Ha below were replaced by “Z”, we’d get a different

diastereomer than we would if Hb were replaced by Z.

• Thus, these two H’s are diastereotopic, and are chemical-shift

inequivalent (i.e., they will each give different 1H NMR signals!). Why? Ha & Hb will always be in different environments; this can be seen if you look at any Newman projection along the C2-C3 bond.

(Note that this molecule is chiral)

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• If Ha below were replaced by “Z”, we’d get a trans isomer; if Hb

were replaced by Z, we’d get a cis isomer--different diastereomers, so Ha and Hb are diastereotopic.

• Note how Ha will always be trans to the CH3, while Hb will

always be cis to it---different environments → different shifts

• The other CH2’s in this thing are all diastereotopic pairs, too!

This may be easier to see in a cyclic case:

Z and CH3 trans Z and CH3 cis

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Q: What is it about a molecule that make it’s CH2’s diastereotopic? A: Generally, this occurs for any molecule with one or more stereocenters, but monosubstituted cycloalkanes and unsymmetrical 1,1-disubstituted alkenes also qualify

stereocenters Ha and Hb are considered diastereotopic

This can complicate 1H NMR spectra significantly. We will see an example on slide 42; the 1H NMR spectrum of

14-20 1H’s of a given type will absorb in a somewhat predictable region:

• 2. Position of Signals--Characteristic Chemical Shifts

Some differences can be explained by electronegativity, but not all….

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• sp2 = “more electronegative” than sp3, but that’s only part of it.
• In a magnetic field, the loosely held  e- of the C=C circulate to

create their own small, induced magnetic field, which reinforces B0 in the vicinity of the H’s.

• a. Alkenes: why are C=C-H’s relatively downfield?
• This is an “anisotropic” effect—the degree and direction of the

shift depend on the location of the H’s within the induced field.

• The alkene H’s are in the “deshielding region” of the C=C.

This moves the 1H signals somewhat downfield (to ~4.5-6.5 ppm).

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• In a magnetic field, the  e- in benzene circulate around the ring

creating a “ring current”—a particularly strong effect.

• The induced field again reinforces B0 in the vicinity of the H’s.
• Thus, the 1H’s again experience a downfield anisotropic effect—
• ften even more so than alkene CH’s ( to ~ 6-8 ppm).
• b. Aromatics? A similar story…

Note: CH’s where the C is connected to the ring (or C=C) will be affected by this, too, but not nearly as much.

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• The  e- of a C≡C also circulate in a magnetic field, but in this

case, the induced field opposes B0 in the vicinity of the C≡C-H.

• Alkyne 1H’s thus absorb relatively upfield (~ 2.5 ppm).
• c. Alkynes?
• Note, however, that hybridization is also a factor—sp orbitals

are more electronegative than sp2 or sp3, so there is a downfield effect mixed in there, too…

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• The chemical shift of almost any kind of C−H usually increases

with increasing alkyl substitution. Q: Hmm—this seems counterintuitive? R-groups are e-- donating, right? Shouldn’t that increase shielding as we go to the right here? What’s the deal? A:  e- circulate, too! The associated fields are weaker, but there are a lot of them. Their effects, together with typical geometric relationships among them, cause this general trend.

• d. Other “Anisotropic” Effects

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Overview of General 1H NMR Spectral Regions

Effects are additive, so these are just approximate ranges. E.g., the CH2O in CH2=CHCH2OH would be a bit further downfield than the one in CH3CH2CH2OH. And, generally,  for CH > CH2 > CH3, given identical substituents.

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• The area of an 1H NMR signal/peak is proportional to the

number of 1H’s associated with it.

• “Integration” of the peak areas is often plotted as a stepped

curve (an integral) above the spectrum.

• The height of each “step” is proportional to the area under

the peak, which is proportional to the number of 1H’s for that signal.

• 3. Intensity of 1H NMR Signals

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• NMR data systems calculate the value of each integral for you

in arbitrary units (or you could just measure with a ruler…).

• The ratio of these values gives info about how many 1H’s of

each type are represented by the various signals.

• This is a ratio—not the absolute number—of 1H’s—but if you

know the molecular formula, you can figure out the numbers.

Ratio of signals is 3:1, but knowing formula (C5H12O), this must translate to 9H:3H If you didn’t know the formula, this’d be tricky to figure out…

3 equivalent CH3’s—one signal for all 9H!

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The text gives another example (C9H10O2; below), but makes things look more complicated than they need to be…

• Their integrals are messed up (e.g., size of integral for A is

clearly not more than twice that for B…??), but…

• Just eyeballing the numbers shown, with an available total of

10H, makes it pretty clear that the ratio must be 5:2:3…

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• 4. Signal Shape: Spin-Spin Coupling/Splitting in 1H NMR
• The simple sample spectra that we have seen up to now have

included only single-peak absorptions called singlets.

• However, signals for individual 1H types often show more

complex shapes, i.e., they are split into more than one peak.

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The reason? Spin-spin coupling (= splitting) generally occurs between non-equivalent 1H’s on the same C or adjacent C’s. Q: Why does the CH2 in BrCH2CHBr2 occur as a doublet?

• When exposed to B0, the adjacent 1H (CHBr2) can be aligned

with () or against () B0.

• Thus, the CH2 can experience two slightly different net

magnetic fields caused by this 1H’s own little field—one slightly larger than B0, and one slightly smaller than B0 (~50:50 chance)

• The corresponding CH2’s absorb at two different frequencies,

so the absorption gets split into a 1:1 doublet.

• As we will soon see, the CH2 will also split the CH signal…

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When two 1H’s split each other, they are said to be coupled. The frequency difference, in Hz, between the two peaks of the doublet is called the coupling constant, J. This “J-value” is a constant and is independent of the B0 being used.

• a. Coupling Constants

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Ok, fine. But why is the CHBr2 signal a 3-line thing (a triplet)?

• When in B0, the adjacent CH2 protons Ha and Hb can each be

aligned with () or against () B0.

• Thus, a CHBr2 proton could experience one of three slightly

different net magnetic fields:

• one slightly larger than B0 (when the CH2 spins are )
• one slightly smaller than B0 (the  case)
• one the same strength as B0 (the  and  cases)
• Because the CHBr2

1H’s can experience 3 different net

magnetic effects, subsets of the population appear at 3 slightly different frequencies, resulting in a triplet.

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• Because there are two ways to align one 1H with B0, and one

against B0 (i.e., ab and ab), the middle peak of the triplet is twice as intense as the two outer peaks.

• This makes the ratio of the areas under the three peaks 1:2:1.
• The distance in Hz between each peak in a simple “multiplet”

like this (i.e., the J-value) will be the same.

With two neighbors Ha and Hb,

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• Some general rules describe splitting patterns commonly

seen in 1H NMR spectra of organic compounds. [1] Equivalent protons do not split each other. [2] A set of n equivalent neighboring 1H’s will split the signal for a nearby 1H type into n + 1 peaks. [3] Splitting is usually observed between non-equivalent 1H’s

• n the same C (geminal H’s) or adjacent C’s (vicinal H’s).
• b. Splitting Patterns

geminal H’s vicinal H’s

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[4] Splitting is not generally observed between 1H’s separated by more than three  bonds. Four-bond couplings can sometimes be seen through - systems, but even these are usually relatively small.

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Another example:

CH3: 3 identical 1H split by 1 adjacent 1H; n + 1 = 2 peaks  doublet CH: 1 1H split by 3 identical adjacent 1H; n + 1 = 4 peaks  “quartet” Quartet is 1:3:3:1 because each 1H

• f the CH3

1H’s could have  or  spin.

All possible combinations will occur, in statistically expected 1:3:3:1 ratio. Often not perfect (as above), but this is the expected ratio.

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1H NMR Spectrum of 2-Bromopropane

• This is a characteristic pattern for an isopropyl group.
• The 6 Ha protons are split by the one Hb to give a doublet.
• Hb is split by 6 equivalent Ha protons to yield a septet (n + 1 = 7).

Relative ratios? From all possible spin combos: 1:6:15:20:15:6:1

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Some other common 1H NMR splitting patterns… Keep in mind the difference between multiplicity and integration…

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• When two different sets of adjacent 1H’s are coupled to a given

1H (n 1H’s on one adjacent C and m 1H’s on another), things

can get more complicated…

• If the J with n = the J with m; the number of peaks in an NMR

multiplet will = (m + n) + 1, as you might have expected.

• However, if the J with n ≠ the J with m, you could see a much

messier multiplet; it could have (m + 1) x (n + 1) lines!

• c. More Complex Splitting Patterns
• Let’s consider these possible

scenarios using an n-propyl group as an example

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Consider the signal for the H2 labelled below as “b”: If Jab = Jbc (or if Jab ≈ Jbc), we’d expect 5 + 1 = 6 peaks/lines for this H2 signal. (We will see this on the next slide…) But…what if Jab is different from Jbc? Just for kicks, let’s say Jab >> Jbc…in that case, we could get 12 lines for that H2 signal!

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• The Hc’s and Ha’s are not equivalent, so we can’t necessarily just

add them together and use the n + 1 rule, but…

• Jab and Jbc tend to be very similar in an open-chain system like

this, so the n + 1 “rule” does work here--the Hb signal is a sextet.

The Actual 1H NMR Spectrum of 1-Bromopropane:

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But here’s one where we do see some different vicinal J-values:

4.0 3.5 3.0 2.5 2.0 1.5 1.0 0.5 0.0

4.1 4.0 3.9 3.8 3.7 3.6 3.5 3.4

The CH2

1H’s are diastereotopic (see slides 17-19), so they are

inequivalent, and appear as two one-H signals ( 3.46 and 3.58). This also makes the CH and CH2 multiplets more complicated! This is a very common phenomenon among compounds that have one or more stereocenters…

Four signals-- integration: 1:1:1:3

TMS

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• 1H’s on C=C’s often give characteristic splitting patterns.

Consider the three possible disubstituted C=C’s…

• When the 1H’s on the C=C are different (usually the case unless

the thing is symmetrical), each 1H splits the signal of the other so that each appears as a doublet (a “d”).

• The magnitude of the J depends on the arrangement of the H’s:
• d. Alkene J-values

This gives us an easy way to tell which kind of system we have!

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Cis vs. trans isomers can easily be distinguished!

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Consider a vinyl group (-CH=CH2). All three H’s are different, and all three possible couplings show up:

vinyl acetate

And the shifts are surprisingly different →

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1H NMR Spectrum of Vinyl Acetate

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• NMR spectra are usually collected using dilute solutions.
• Regular solvents pose a problem--so much more abundant

than the analyte that they would give giant masking signals…

• Solution: deuterated solvents—classic example = CDCl3 (as
• pposed to CHCl3). D (= 2H) does not show a 1H NMR signal!
• Could still see a small CHCl3 signal (~7.26 ppm), but it is due to

trace residual CHCl3, not the CDCl3.

• e. NMR Solvents

7.5 7.0 6.5 6.0 5.5 5.0 4.5 4.0 3.5 3.0 2.5 2.0 1.5 1.0 0.5

solvent peak TMS (standard) Analyte signals

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• OH (and amine NH) protons behave differently from CH’s,

mainly because they undergo H-bonding and/or exchange.

• An OH might not show coupling with adjacent CH’s (as below),

but for another sample of the same compound, it might!

• Consider the spectrum of ethanol (CH3CH2OH) below:
• f. 1H NMR Signals for OH Protons

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• The three-proton CH3 signal is split by the CH2 into a triplet.
• The two-proton CH2 signal is split by the CH3 into a quartet.
• But…the adjacent OH shows no coupling with the CH2???
• OH’s often undergo intermolecular exchange so rapidly that a

given OH proton is not around long enough to exert mutual spin effects with the CH2 → no coupling!

• If rate is slowed somehow (e.g., in very dilute solution),

coupling can sometimes be seen, but this is hard to predict.

• Intermediate situations can occur where coupling is not
• bserved, but the OH shows up as a broad lump…can even

be so broad that you don’t notice it!

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• Cyclohexane conformers interconvert rapidly at room
• temperature. An NMR spectrum shows an average of these.
• Each C has two different types of H—one axial, one equatorial—

but their rapid interconversion results in a single NMR signal due to the average environment that each H experiences.

• g. Cyclohexane Conformers
• Otoh, if a system has a strongly preferred conformer, e.g., due to

a t-butyl substituent, then the ax and eq H’s would be different.

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• Benzene’s 1H’s are equivalent, and give one peak at 7.27 ppm.
• Monosubstituted benzenes contain five 1H’s that are not all

equivalent; the appearance of the signals varies, depending

• n what is attached.
• h. Protons on Benzene Rings

Think about why this might be—we’ll revisit it when we talk more about benzenes…

Patterns for more highly substituted benzenes will be diagnostic because their vicinal J-values are larger (ca. 7.5 Hz) than others.

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• i. Overlapping signals
• Efforts (even counting signals) can be hampered by overlap of

signals that have very similar chemical shifts.

• For example, technically, 1-chlorooctane (below) has eight

different kinds of H. (This is what the book would say…)

• However, the environments of some of the CH2’s are so similar

that they resonate at about the same place, giving a nearly uninterpretable blob with confusing integration…

3.5 3.0 2.5 2.0 1.5 1.0 0.5 0.0

Still get some useful info

• ut of it, but this does

complicate things…

2H 2H 3H

TMS

C8H17Cl

10H (!)

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• H. Use of 1H NMR in Structure Determination

1. Figure the number of unsaturations: #C – ½ #(H + X) + ½ #N + 1 2. Count the signals: try to determine the # of different types of H 3. Look at integration to tell how many of each type you have. This can tell you whether a signal = a CH3 or a CH or CH2. Think about possible symmetry issues.

• 4. Look at splitting to tell what’s next to what. Look for

diagnostic patterns (e.g., see slide 38).

• 5. Consider chemical shifts (and any other available information,

such as IR) to decide what kind of functional groups you might have, and which H’s they are near. Some steps to consider are listed below. They do not have to be followed in this order. With practice, some will become intuitive.

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Example: C4H8O2; IR says there’s a C=O

• 1. Number of unsaturations = 4 – 4 + 1 = 1 (the C=O must be the
• nly one!)
• 2. Number of different types of H? There are three (three signals).

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• 3. How many of each type (based on integration)? Ratio of 3:2:3

(and 3H + 2H + 3H = 8H; matches formula). (Only 4 C → this must correspond to two CH3’s and a CH2). So…we have a C=O, two different CH3’s, a CH2, and one more O. Not all that many possibilities….but let’s keep going…

• 4. Splitting? CH3 at 1.1 ppm and CH2 split each other → an

ethyl pattern, just like in ethanol. The other CH3 is a singlet— it must have no vicinal H neighbors!

• 5. Shift—at this point, there are only two chemically reasonable

structures, and shift distinguishes them: The only way the CH3 singlet can be downfield of the CH2 is to place it on the electronegative O

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• 12C is not NMR-active because its I value = 0.
• However, 1.1% of the carbon nuclei in nature are not 12C—they

are 13C (remember that from the MS chapter?), and the I value for 13C = ½, just like 1H, so we can see 13C’s by NMR!

• “Standard” 13C NMR spectra are easier to analyze because the

signals are not split; each type of C appears as a single peak.

• G. 13C NMR Spectra
• Huh? Why should

that be??

• Two reasons…

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The 13C’s out there are randomly distributed among all possible positions within a molecule. Due to its low natural abundance (1.1%), the chance of two 13C’s being bonded to each other is very small (0.011 x 0.011 = 0.0001%) Thus, nearly all 13C’s will be attached to NMR-inactive 12C, which does not cause splitting. Q: But couldn’t 13C NMR signals be split by nearby 1H’s? A: Yes, but standard 13C NMR experiments employ a technique that “decouples” the 1Hs from the 13C’s, so that every 13C peak is simplified to a singlet. This throws away coupling information, and prevents accurate integration, but makes the thing easier to interpret AND improves s/n (remember, we can only see 1% of the carbons in the sample…)

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Since we don’t see the coupling and can’t integrate, there are

• nly two features of a standard 13C NMR spectrum that provide

structural info:

• Number of signals: indicates the number of “different types
• f C” (i.e., different environments of C’s) in a molecule.
• Position of signals: shifts help sort out what types of C the

molecule contains.

• H. Types of Structural Info Provided by 13C NMR Spectra

Re intensities: we can’t accurately integrate 13C NMR spectra, but signals that correspond to more than one identical C (e.g., the CH3 in (CH3)2CHOH) do tend to be somewhat larger. Also, C’s with no H on them tend to give somewhat smaller signals than others.

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• 1. Number of signals

Recognizing the # of different types of C has analogy to the spotting the # of different types of H. However, must be wary of symmetry issues…e.g., the compound below would have only four 13C NMR signals in the sp2 region (plus the OCH3 carbon in the sp3 region):

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• 13C NMR signals occur over a much broader chemical shift

range than 1H signals (ca. 0-220 ppm downfield from TMS).

• Why? C’s can be hybridized differently—H cannot—and each C

is bonded to more things than an H. There’s just more variety….

• Chemical shift trends in 13C NMR parallel those in 1H NMR,

because the same basic kinds of factors influence them.

• 2. Position—chemical shift range

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13C NMR Spectrum

• f 1-Propanol:

13C NMR Spectrum

• f Methyl Acetate:

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An advantage of the wide shift range and sharp signals is that

13C NMR spectra tend to have less of an issue with overlap.

Remember that blobby 1H NMR spectrum of 1-chlorooctane on slide 52? The 13C NMR spectrum clearly resolves all eight 13C signals!

C8H17Cl

55 50 45 40 35 30 25 20 15 10 5

TMS

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• Thus, 13C NMR is a useful compliment to 1H NMR in structure

determination.

• Allows C-types to be counted, and shows signals for C’s that

do not have 1H on them.

• e.g., 1H NMR alone would not explicitly show you that you

have a C=O, but 13C NMR would...

• There are many other, more sophisticated NMR techniques

available to help deal with more complicated structures, but they are beyond the scope of this course.

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A Final NMR Note--Magnetic Resonance Imaging (MRI)

MRI—a valuable technique used in medicine for visualizing soft tissues not well resolved by x-rays—employs NMR technology, but note how they avoided using the term “nuclear”...

an MRI instrument an image showing an area of compression (box A) in a spinal column